A mechanism of coronal transients for material injected into streamer.

Details A mechanism of coronal transients for material injected into streamer. A mechanism of coronal transients for material injected into streamer.

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983acasn..24..401h&link_type=abstract

Acta Astron. Sin., Vol. 24, No. 4, p. 401 - 409

Astronomy and Astrophysics

Astronomy

1

Solar Coronal Transients

Scientific paper

The region of high plasma density may be formed with the streamer configuration, when the dense plasma injects into the coronal local region with open magnetic field. In the present paper, the observational features of the coronal transient of material injected into streamer are summarized. Then the author solves the unsteady, two-dimensional gasdynamical equations. The similarity solutions are given for the typical flow field. The flow features and the profiles of thermodynamical quantities of the similarity solutions agree qualitatively with the observational features. Finally, different configurations of the coronal transient are explained by the dense plasma injecting into different configurations of the magnetic field.

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